High resolutions studies of the structure of the solar atmosphere

Details High resolutions studies of the structure of the solar atmosphere High resolutions studies of the structure of the solar atmosphere

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sao..reptr....h&link_type=abstract

Annual Report No. 1, 1 Jul. 1991 - 30 Jun. 1992 Smithsonian Astrophysical Observatory, Cambridge, MA.

Physics

High Resolution, Image Enhancement, Image Processing, Research And Development, Solar Activity, Solar Atmosphere, Solar Corona, Solar Heating, Stellar Physics, China, University Program

Scientific paper

During this first year, we have concentrated on the analysis, and the
image enhancement and processing of an extensive set of the EUV/Skylab
data for the search of empirical characteristics of coronal heating in
different scale magnetic regions on the Sun. Student involvement in our
research projects has been quite successful.

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